Vestiges of the Natural History of CreationChambers, Robert
Science
Vestiges of the Natural History of Creation
Chambers, Robert
Creation; Evolution (Biology)
Such is an outline of the information which chemistry gives us regarding
the constituent materials of our globe. How infinitely is the knowledge
increased in interest, when we consider the probability of such being the
materials of the whole of the bodies of space, and the laws under which
these everywhere combine, subject only to local and accidental
variations!
In considering the cosmogenic arrangements of our globe, our attention is
called in a special degree to the moon.
In the nebular hypothesis, satellites are considered as masses thrown off
from their primaries, exactly as the primaries had previously been from
the sun. The orbit of any satellite is also to be regarded as marking
the bounds of the mass of the primary at the time when that satellite was
thrown off; its speed likewise denotes the rapidity of the rotatory
motion of the primary at that particular juncture. For example, the
outermost of the four satellites of Jupiter revolves round his body at
the distance of 1,180,582 miles, shewing that the planet was once
3,675,501 miles in circumference, instead of being, as now, only 89,170
miles in diameter. This large mass took rather more than sixteen days
six hours and a half (the present revolutionary period of the outermost
satellite) to rotate on its axis. The innermost satellite must have been
formed when the planet was reduced to a circumference of 309,075 miles,
and rotated in about forty-two hours and a half.
From similar inferences, we find that the mass of the earth, at a certain
point of time after it was thrown off from the sun, was no less than
482,000 miles in diameter, being sixty times what it has since shrunk to.
At that time, the mass must have taken rather more than twenty-nine and a
half days to rotate, (being the revolutionary period of the moon,)
instead of as now, rather less than twenty-four hours.
The time intervening between the formation of the moon and the earth’s
diminution to its present size, was probably one of those vast sums in
which astronomy deals so largely, but which the mind altogether fails to
grasp.
Public-domain text, read in full here on John Shaqi.
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